Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy

Abstract

The unifying approach to early-time and late-time universe based on phantom cosmology is proposed. We consider gravity-scalar system which contains usual potential and scalar coupling function in front of kinetic term. As a result, the possibility of phantom-non-phantom transition appears in such a way that universe could have effectively phantom equation of state at early time as well as at late time. In fact, the oscillating universe may have several phantom and non-phantom phases. As a second model we suggest generalized holographic dark energy where infrared cutoff is identified with combination of FRW parameters: Hubble constant, particle and future horizons, cosmological constant and universe life-time (if finite). Depending on the specific choice of the model the number of interesting effects occur: the possibility to solve the coincidence problem, crossing of phantom divide and unification of early-time inflationary and late-time accelerating phantom universe. The bound for holographic entropy which decreases in phantom era is also discussed.

13 pages, clarifications/refs added, to match with published version

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• $f(R)$ Dual Theories of Quintessence : Expansion-Collapse Duality
• The dressing procedure for the cosmological equations and the indefinite future of the universe
• Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe
• Tsallis holographic dark energy model with event horizon cutoff in modified gravity
• Second order invariants and holography
• Transient dark energy, cosmological constant boundary crossing and dark energy $w(z)$ data fits
• Cosmic Steps in Modeling Dark Energy
• Holographic Principle, Cosmological Constant and Cyclic Cosmology
• Interacting and Non-interacting Reńyi Holographic Dark Energy Models in DGP Braneworld
• Eternal vs singular observers in interacting dark energy-dark matter models
• Constraints on Generalized Gravity-Thermodynamic Cosmology from DESI DR2
• A closer look at the cosmological implications of the $\Lambda$HDE model
• Non-Gaussianity from Features
• Power Law and Logarithmic Ricci Dark Energy Models in Horava-Lifshitz Cosmology
• Gauss-Bonnet Braneworld Cosmology with Modified Induced Gravity on the Brane
• Reexamining RHDE Models in FRW Universe with two IR cut-off with redshift parametrization
• Generalized Holographic Cosmology: low-redshift observational constraint
• Analysis on a General Class of Holographic Type Dark Energy Models
• Analytic solution and Noether symmetries for the hyperbolic inflationary model in the Jordan frame
• Thermodynamics of the most generalized form of Holographic Dark Energy and some particular cases with Corrected Entropies
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Rips and regular future scenario with Holographic Dark Energy: A comprehensive look
• The generalized second law of thermodynamics of the universe bounded by the event horizon and modified gravity theories
• A comprehensive analysis of Barrow holographic Chaplygin gas model reconstruction and its cosmological consequences
• Implementation of cosmological bounce inflation with Nojiri-Odintsov generalized holographic dark fluid
• New method of exponential potentials reconstruction based on given scale factor in phantonical two-field models
• The Holographic cosmology with axion field
• A class of regular bouncing cosmologies
• Holographic description of unified early and late universe in viscous mimetic gravity
• Anisotropic cosmology using observational datasets: exploring via machine learning approaches
• Holographic bounce cosmological models induced by viscous dark fluid from a generalized non-singular entropy function
• Sequestering Mechanism in Scalar-Tensor Gravity
• Inflation via logarithmic entropy-corrected holographic dark energy model
• Qualitative behaviour of higher-curvature gravity with boundary terms i.e the f(Q) gravity models by dynamical system analysis
• Power-law expansion and Higgs-type potential in a scalar-tensor model
• G-corrected holographic dark energy model
• Space-time uncertainty relation from quantum and gravitational principles
• Cosmology in holographic non-minimal derivative coupling theory: constraints from inflation and variation of gravitational constant
• A Cosmological Holographic Reconstruction of f(Q) Theory
• Holographic description of the dissipative unified dark fluid model with axion field
• Holographic F(Q,T) Gravity with Lambert Solution
• Phase space analysis of a FRW cosmology in the Maxwell$-$Cattaneo approach
• Anisotropic power-law inflation for the Sáez-Ballester theory non-minimally coupled to a vector field
• Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
• Revisiting Holographic Dark Energy in Cyclic Cosmology
• Einstein static universe, GUP, and natural IR and UV cut-offs
• Holographic description of the dissipative model of universe with curvature
• Geometric sigma model of the Universe
• A non-singular closed bouncing universe without violation of null energy condition
• Cosmological Constraints on 4D Einstein-Gauss-Bonnet Gravity and Kaniadakis Holographic Dark Energy: Implications for Black Hole Shadows
• f(R) cosmological solutions with varying speed of light
• Ricci-Cubic Holographic Dark Energy: Confronting Observations, Stability and the Cosmic Coincidence Problem
• Qualitative analysis of a quasi-magnetic universe
• Towards the unification of late-time acceleration and inflation by k-essence model
• Kinematic equivalence between models driven by DBI field with constant $\gamma$ and exotic holographic quintessence cosmological models
• Reheating via gravitational particle production in simple models of quintessence or $\Lambda$CDM inflation
• Evolution of the horizons for dark energy universe
• Holographic description of $F(R)$ gravity coupled with Axion Dark Matter
• The Coincidence Problem in Holographic f(R) Gravity
• "Microscopic" approach to the Ricci dark energy
• Holographic Ricci DE as running vacuum with nonlinear interactions
• Rényi Holographic Dark Energy Models In Multidimensional Universe
• Kaniadakis holographic dark energy: observational constraints and global dynamics
• An exotic k-essence interpretation of interactive cosmological models
• Observational Constraints on Chaplygin Gas Models in Non-Minimally Coupled Power Law $f(Q)$ Gravity with Quasars
• Dynamics of Linear Scalar Perturbation in f(Q)+f(T) class of f(Q,T) gravity
• Perturbations In Some Dark Energy Models
• A Combined Barrow Entropy and QCD Ghost Mechanism for Late-Time Cosmic Acceleration
• First-order phase transitions and cosmic evolution: thermodynamic approach to generalized holographic dark energy
• Holographic cosmic energy, fundamental physics and the future of the universe
• The long freeze: an asymptotically static universe from holographic dark energy
• Impact of the Infrared Cutoff on Structure Formation in Tsallis Holographic Dark Energy
• Power-law holographic dark energy and cosmology
• Holographic dark energy models with Interactions and entropy corrections for different cutoffs in the Brans-Dicke cosmology
• Linearly Interacting Barrow Holographic Dark Energy in Modified Cosmology
• Confronting phantom inflation with Planck data
• Study of Tachyonic Field and its statefinder diagnostics in Various Scenarios of The Anisotropic Universe
• Entropy-Corrected New Agegraphic Dark Energy Model in Horava-Lifshitz Gravity
• Scalar-Field Reconstruction of Ricci--Gauss--Bonnet Dark Energy in Hořava--Lifshitz Cosmology
• Quintessence reconstruction of interacting HDE in a non-flat universe
• Dark energy and the future fate of the Universe